Search Results
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bundle:
Quasi Thermal Noise pectroscopy on High Frequency Receiver Data Bundle
This bundle contains RPWS-HFR Quasi Thermal Noise (QTN) spectroscopy supplied CDF and plot files containing a time series of thermal plasma moments (density and temperature). QTN data products are generated only when the QTN analysis is applicable. -
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VIMS Observations from the Cassini Cruise to Saturn
This bundle contains Cassini VIMS data, metadata, and associated documentation from the cruise to Saturn--October 1997 through December 2003. -
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VIMS Observations from the Cassini Tour of the Saturn System
This bundle contains Cassini VIMS data, metadata, and associated documentation for the Saturn tour--January 2004 through end of mission in September 2017. -
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GASKELL DIONE SHAPE MODEL
The shape model of Dione derived by Robert Gaskell from Cassini images. The model is provided in the implicitly connected quadrilateral (ICQ) format. This version of the model was prepared on July 23, 2012. Vertex-facet versions of the models are also provided. -
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GASKELL MIMAS SHAPE MODEL
The shape model of Mimas derived by Robert Gaskell from Cassini ISSNA and ISSWA images and Voyager 1 ISSN images. The model is provided in the implicitly connected quadrilateral (ICQ) format. This version of the model was prepared on June 26, 2012. Vertex-facet versions of the models are also provided. -
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ISS Observations from the Cassini Cruise to Saturn
This bundle contains Cassini ISS images, metadata, and associated documentation from the cruise to Saturn--October 1997 through December 2003. -
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GASKELL PHOEBE SHAPE MODEL
The shape model of Phoebe derived by Robert Gaskell from Cassini images. The model is provided in the implicitly connected quadrilateral (ICQ) format. This version of the model was prepared on August 4, 2012. Vertex-facet versions of the models are also provided. -
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ISS Observations from the Cassini Tour of the Saturn System
This bundle contains Cassini ISS images, metadata, and associated documentation for the Saturn tour--January 2004 through end of mission in September 2017. -
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CASSINI HIGH RATE DETECTOR
The High Rate Detector (HRD) from the University of Chicago is an independent part of the CDA instrument on the Cassini Orbiter that measures the dust flux and particle mass distribution of dust particles hitting the HRD detectors. This data set includes all data from the HRD through the end of the mission, Sept. 15, 2017. Please refer to Srama et al. (2004) for a detailed HRD description. -
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GASKELL TETHYS SHAPE MODEL
The shape model of Tethys derived by Robert Gaskell from Cassini Imaging Science Subsystem narrow and wide angle camera (ISSNA and ISSWA) images. The model is provided in the implicitly connected quadrilateral (ICQ) format. This version of the model was prepared on July 25, 2012. Vertex-facet versions of the models are also provided. -
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Cassini RPWS Electron Densities from Upper Hybrid and Plasma Wave Frequencies
This bundle provides electron number density values derived from features observed in plasma wave data obtained by the Cassini Radio and Plasma Wave Science (RPWS) instruments, along with observed or derived characteristic frequencies, and useful positional parameters for the spacecraft and related bodies. When present, frequency values of narrowband emissions at the upper hybrid resonance were digitized and combined with measured or model magnetic field to derive electron number density. At other times, features such as the upper cutoff in auroral hiss or electron plasma oscillations were used to determine the plasma frequency and electron density.
Data Sets and Information